Motivated by the apparent dependence of string –models on the sum of
spacetime metric and antisymmetric tensor fields, we reconsider gravity
theories constructed from a nonsymmetric metric. We first show that all such
“geometrical” theories homogeneous in second derivatives violate standard
physical requirements: ghost-freedom, absence of algebraic inconsistencies or
continuity of degree-of-freedom content. This no-go result applies in
particular to the old unified theory of Einstein and its recent avatars.
However, we find that the addition of nonderivative, cosmological'' terms formally restores consistency by giving a mass to the antisymmetric tensor field, thereby transmuting it into a fifth-force-like massive vector but with novel possible matter couplings. The resulting macroscopic models also exhibit van der Waals’'-type gravitational effects, and may provide useful
phenomenological foils to general relativity.

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